<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-06-23T03:48:16Z</responseDate><request verb="GetRecord" identifier="oai:riubu.ubu.es:10259/7222" metadataPrefix="mods">https://riubu.ubu.es/oai/request</request><GetRecord><record><header><identifier>oai:riubu.ubu.es:10259/7222</identifier><datestamp>2023-03-24T13:07:23Z</datestamp><setSpec>com_10259.4_2557</setSpec><setSpec>com_10259_5086</setSpec><setSpec>com_10259_2604</setSpec><setSpec>col_10259_7221</setSpec></header><metadata><mods:mods xmlns:mods="http://www.loc.gov/mods/v3" xmlns:doc="http://www.lyncode.com/xoai" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.loc.gov/mods/v3 http://www.loc.gov/standards/mods/v3/mods-3-1.xsd">
<mods:name>
<mods:namePart>Gubitosi, Giulia</mods:namePart>
</mods:name>
<mods:name>
<mods:namePart>Ballesteros Castañeda, Ángel</mods:namePart>
</mods:name>
<mods:name>
<mods:namePart>Herranz Zorrilla, Francisco José</mods:namePart>
</mods:name>
<mods:extension>
<mods:dateAvailable encoding="iso8601">2023-01-09T11:55:21Z</mods:dateAvailable>
</mods:extension>
<mods:extension>
<mods:dateAccessioned encoding="iso8601">2023-01-09T11:55:21Z</mods:dateAccessioned>
</mods:extension>
<mods:originInfo>
<mods:dateIssued encoding="iso8601">2020-08</mods:dateIssued>
</mods:originInfo>
<mods:identifier type="issn">1824-8039</mods:identifier>
<mods:identifier type="uri">http://hdl.handle.net/10259/7222</mods:identifier>
<mods:identifier type="doi">10.22323/1.376.0190</mods:identifier>
<mods:abstract>Given a group of kinematical symmetry generators, one can construct a compatible noncommutative spacetime and deformed phase space by means of projective geometry. This was the main&#xd;
idea behind the very first model of noncommutative spacetime, proposed by H.S. Snyder in 1947.&#xd;
In this framework, spacetime coordinates are the translation generators over a manifold that is&#xd;
symmetric under the required generators, while momenta are projective coordinates on such a&#xd;
manifold. In these proceedings we review the construction of Euclidean and Lorentzian noncommutative Snyder spaces and investigate the freedom left by this construction in the choice of the&#xd;
physical momenta, because of different available choices of projective coordinates. In particular,&#xd;
we derive a quasi-canonical structure for both the Euclidean and Lorentzian Snyder noncommutative models such that their phase space algebra is diagonal although no longer quadratic.</mods:abstract>
<mods:language>
<mods:languageTerm>eng</mods:languageTerm>
</mods:language>
<mods:accessCondition type="useAndReproduction">http://creativecommons.org/licenses/by-nc-nd/4.0/</mods:accessCondition>
<mods:accessCondition type="useAndReproduction">info:eu-repo/semantics/openAccess</mods:accessCondition>
<mods:accessCondition type="useAndReproduction">Attribution-NonCommercial-NoDerivatives 4.0 Internacional</mods:accessCondition>
<mods:titleInfo>
<mods:title>Generalized noncommutative Snyder spaces and projective geometry</mods:title>
</mods:titleInfo>
<mods:genre>info:eu-repo/semantics/conferenceObject</mods:genre>
</mods:mods></metadata></record></GetRecord></OAI-PMH>